High ionization lines (HIL; IP\(>\) 40 eV), Civ\(\lambda \) 1549, Heii\(\lambda \) 1640 and Siiv\(\lambda \) 1397, show a prominent blueshifted component. We find that the blue component has a contribution of 76\(\%\) , 62\(\%\)  and 57\(\%\)  to the total flux of Civ\(\lambda \) 1549, Heii\(\lambda \) 1640 and Siiv\(\lambda \) 1397 respectively. The Civ\(\lambda \) 1549 reaches c(\({1}{2})\sim \) –6000\(\pm \) 500 km s\(^{-1}\) , while Heii\(\lambda \) 1640 and Siiv\(\lambda \) 1397 c(\({1}{2})\sim \) –4000\(\pm \) 550 km s\(^{-1}\) . The velocities reached are ones of the highest found in the literature [1]}, [2]}, [3]}. Then, it indicates that the full profile is dominated by an outflow and suggests the disk plus wind scenario [4]}, [5]}, [1]}.
